What happens when gamma rays with ultra-high energies interact with matter?

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SUMMARY

The discussion centers on the interactions of ultra-high energy gamma rays with matter, specifically focusing on the dominance of pair production processes over other interactions such as photoelectric and Compton scattering. As gamma ray energy increases, various absorption channels open, including photonuclear reactions at around 10 MeV and pion production at 140 MeV. The conversation highlights that while pair production remains dominant even at energies exceeding 2 TeV, other processes like muon pair production and photon-gluon fusion, although rare, become relevant at very high energies. The Bethe-Heitler process is noted for its significant disparity in production rates between muons and electrons.

PREREQUISITES
  • Understanding of gamma ray interactions with matter
  • Familiarity with pair production and its significance in high-energy physics
  • Knowledge of photonuclear reactions and their energy thresholds
  • Basic principles of quantum chromodynamics (QCD) and electromagnetic processes
NEXT STEPS
  • Research the mechanisms of photonuclear reactions and their energy thresholds
  • Study the Bethe-Heitler process and its implications in high-energy physics
  • Explore the role of photon-gluon fusion in particle interactions
  • Investigate the production rates of various particle pairs at high energies
USEFUL FOR

Physicists, researchers in high-energy particle physics, and students studying gamma ray interactions and quantum mechanics will benefit from this discussion.

neanderthalphysics
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What sort of properties would you expect from gamma rays, as you increase their energy, and why? Would they penetrate high Z-matter more easily? What would be the outcome of the interactions? Do you expect photoelectric and Compton scattering processes to become negligible, and the dominant interaction mechanism becomes pair production?

On a macroscopic scale, what do you think would happen if photons with energies of something like 1J each interacts with matter? A very small antimatter explosion from pair production and subsequent annihilation?
 
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Pair production is dominant already at the GeV range and it stays that way. You get electromagnetic showers with electrons, positrons and photons. Towards the end you get more and more lower energy processes.
 
As the energy increases, you have additional absorption channels opening up:
  • Around 10 MeV depending on the target nuclei - photonuclear reactions
  • About 140 MeV - direct pion production
  • About 210 MeV - muon pair production
  • About 300 MeV - a resonance peak of pion production via Δ
  • About 700 MeV - start of hyperon production, like p+γ→Λ+K+
  • About 1900 MeV - nucleon pair production, and soon after hyperon pairs
  • About 3500 MeV - tauon pair production, and soon after charm
  • Around 10 GeV - beauty pair production
  • From 80 GeV - real W and soon after Z bosons.
Is it confirmed that simple electron-positron pair production stays dominant above all the higher energy processes combined at all energies, including their resonance peaks/edges?
 
We have photons up to ~2 TeV in the LHC collisions. They make electromagnetic showers as expected. The other processes are not impossible but very rare. Resonances are rare or very narrow, the latter makes them rare for a relevant photon spectrum.
Some of your thresholds are too low, by the way. An 80 GeV photon hitting a nucleus doesn't have 80 GeV center of mass energy with the photon/quark system, it only has something of the order of 10 or even less.
 
mfb said:
Some of your thresholds are too low, by the way.

All of them besides the one where "it depends". (And there is no such thing as a "tauon".)

mfb said:
The other processes are not impossible but very rare.

True, but I don't think that gets across how rare is rare. The Bethe-Heitler process goes as 1/m2 so muon pair production at very high energies is 1/40,000 of the electron rate. There's also threshold effects at low and moderate energies: 99.998% of 500 MeV photons don't produce muons.

Even correcting the errors, these additional processes just aren't relevant.

The process that becomes relevant at very high energies is photon-gluon fusion, because that happens with QCD-sized cross-sections, not EM-sized cross-sections. This is still rare: say the 1/1000 rate instead of the 1/100,000+ you might expect from a pure EM process.
 
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